Airfix A11170 Apollo Saturn V 1:144 Scale Series 11 Plastic Model Kit

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Melosh, H. Jay (2011). Planetary Surface Processes. Cambridge Planetary Science. Vol.13. Cambridge University Press. p.5. ISBN 978-0-521-51418-7. Archived from the original on 16 February 2017 . Retrieved 9 February 2016. a b Mankovich, Christopher; etal. (17 January 2019). "Cassini Ring Seismology as a Probe of Saturn's Interior. I. Rigid Rotation". The Astrophysical Journal. 871 (1): 1. arXiv: 1805.10286. Bibcode: 2019ApJ...871....1M. doi: 10.3847/1538-4357/aaf798. S2CID 67840660. Hanel, R.A.; etal. (1983). "Albedo, internal heat flux, and energy balance of Saturn". Icarus. 53 (2): 262–285. Bibcode: 1983Icar...53..262H. doi: 10.1016/0019-1035(83)90147-1. a b Schmude, Richard W. Jr. (Winter 2003). "Saturn in 2002–03". Georgia Journal of Science. 61 (4). ISSN 0147-9369. Archived from the original on 24 September 2015 . Retrieved 29 June 2015. Pioneer 11 made the first flyby of Saturn in September 1979, when it passed within 20,000km of the planet's cloud tops. Images were taken of the planet and a few of its moons, although their resolution was too low to discern surface detail. The spacecraft also studied Saturn's rings, revealing the thin F-ring and the fact that dark gaps in the rings are bright when viewed at a high phase angle (towards the Sun), meaning that they contain fine light-scattering material. In addition, Pioneer 11 measured the temperature of Titan. [159] Voyager flybys

Saturn occupies almost 60 percent of Jupiter’s volume but has only about one-third of its mass and the lowest mean density—about 70 percent that of water—of any known object in the solar system. Hypothetically, Saturn would float in an ocean large enough to hold it. Both Saturn and Jupiter resemble stars in that their bulk chemical composition is dominated by hydrogen. Also, as is the case for Jupiter, the tremendous pressure in Saturn’s deep interior maintains the hydrogen there in a fluid metallic state. Saturn’s structure and evolutionary history, however, differ significantly from those of its larger counterpart. Like the other giant, or Jovian, planets—Jupiter, Uranus, and Neptune—Saturn has extensive systems of moons (natural satellites) and rings, which may provide clues to its origin and evolution as well as to those of the solar system. Saturn’s moon Titan is distinguished from all other moons in the solar system by the presence of a significant atmosphere, one that is denser than that of any of the terrestrial planets except Venus. Godfrey, D. A. (1988). "A hexagonal feature around Saturn's North Pole". Icarus. 76 (2): 335. Bibcode: 1988Icar...76..335G. doi: 10.1016/0019-1035(88)90075-9.Pence, Michael (9 March 2006). "NASA's Cassini Discovers Potential Liquid Water on Enceladus". NASA Jet Propulsion Laboratory. Archived from the original on 11 August 2011 . Retrieved 3 June 2011. a b "Missions to Saturn". The Planetary Society. 2007. Archived from the original on 28 July 2011 . Retrieved 24 July 2007. In March 2007, it was found that the variation in radio emissions from the planet did not match Saturn's rotation rate. This variance may be caused by geyser activity on Saturn's moon Enceladus. The water vapor emitted into Saturn's orbit by this activity becomes charged and creates a drag upon Saturn's magnetic field, slowing its rotation slightly relative to the rotation of the planet. [94] [95] [96] Saturn's Known Satellites". Department of Terrestrial Magnetism. Archived from the original on 26 September 2011 . Retrieved 22 June 2010. NASA: Solar System Exploration: Planets: Saturn: Facts & Figures". Solarsystem.nasa.gov. 22 March 2011. Archived from the original on 2 September 2011 . Retrieved 8 August 2011.

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Scientists Find That Saturn's Rotation Period is a Puzzle". NASA. 28 June 2004. Archived from the original on 29 July 2011 . Retrieved 22 March 2007. Shiga, David (20 September 2007). "Faint new ring discovered around Saturn". NewScientist.com. Archived from the original on 3 May 2008 . Retrieved 8 July 2007. Cain, Fraser (22 January 2009). "Atmosphere of Saturn". Universe Today. Archived from the original on 12 January 2012 . Retrieved 20 July 2011. General Information About Saturn". Scienceray. 28 July 2011. Archived from the original on 7 October 2011 . Retrieved 17 August 2011.Strongest evidence yet indicates Enceladus hiding saltwater ocean". Physorg. 22 June 2011. Archived from the original on 19 October 2011 . Retrieved 19 July 2011. Many of the other moons are small: 131 are less than 50km in diameter. [105] Traditionally, most of Saturn's moons have been named after Titans of Greek mythology. Titan is the only satellite in the Solar System with a major atmosphere, [106] [107] in which a complex organic chemistry occurs. It is the only satellite with hydrocarbon lakes. [108] [109] Gurnett, D. A.; etal. (2007). "The Variable Rotation Period of the Inner Region of Saturn's Plasma Disc" (PDF). Science. 316 (5823): 442–5. Bibcode: 2007Sci...316..442G. doi: 10.1126/science.1138562. PMID 17379775. S2CID 46011210. Archived from the original (PDF) on 12 February 2020. Chang, Kenneth (14 September 2017). "Cassini Vanishes Into Saturn, Its Mission Celebrated and Mourned". The New York Times. Archived from the original on 8 July 2018 . Retrieved 15 September 2017.